A Stochastic Approach to Reconstruct Gamma-Ray-burst Light Curves

Gamma-ray bursts (GRBs), as they are observed at high redshift ( z = 9.4), are vital to cosmological studies and investigating Population III stars.To tackle these studies, we need correlations among relevant GRB variables with the requirement Accessories of small uncertainties on their variables.Thus, we must have good coverage of GRB light curves

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